A long hard look at the minimum state of PG 2112+059 with XMM-Newton

Astronomy and Astrophysics

Volumn 512, Issue 12, 2010, Pages

  Schartel, N ^a   Rodriguez Pascual P M ^a   Santos Lleo M ^a   Jimenez Bailon E ^b   Ballo, L ^a,c   Piconcelli, E ^d  

^a EUROPEAN SPACE AGENCY   (Spain)

^b UNIVERSIDAD NACIONAL AUTÓNOMA DE MÉXICO   (Mexico)

^c INSTITUTO DE FÍSICA DE CANTABRIA CSIC UC   (Spain)

^d INAF OSSERVATORIO ASTRONOMICO DI ROMA   (Italy)

Author keywords

Galaxies: active; Quasars: individual: PG 2112+059

Indexed keywords

DISKS (STRUCTURAL COMPONENTS); GALAXIES; IONIZATION; X RAY ANALYSIS; X RAY SPECTROGRAPHS;

ACCRETION DISKS; BLACK HOLES; CHANDRA; COLUMN DENSITY; EMISSION LINES; EMISSION SCENARIO; GALAXIES : ACTIVE; INTRINSIC EMISSION; IONISATION; LIGHT-BENDING; QUASARS: INDIVIDUAL; SELF-CONSISTENCY; SIGNAL TO NOISE; SPECTRAL VARIABILITY; TWO LAYERS; X-RAY EMITTING; X-RAY OBSERVATIONS; X-RAY SPECTRA; XMM-NEWTON;

REFLECTION;

EID: 77951579486     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/200912389     Document Type: Article

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